3 General Topics in Geochemistry

Sunday, 21 April 2024
1:30 PM - 5:30 PM
Coco Ballroom, Oasis CC


WORKING TOWARDS A COMPREHENSIVE DIAGENETIC MODEL FOR IRON-RICH SEDIMENTARY ROCKS

Paper number: 3-1
Program: Theme Sessions
Time: 1:30 PM – 1:50 PM


Authors


Abstract

Some geochemical proxies hint at a prolonged interval of low or unstable surface oxygen levels across the Proterozoic following the Great Oxidation Event. Primary mineral phases in chemical sedimentary rocks archive seawater geochemistry across these critical geologic intervals. However, uncertainties in the effects of diagenesis and other post-depositional changes on proxy records complicate the reconstruction of geochemical attributes of evolving Proterozoic environments. A mineral reaction database that catalogs depositional vs. post-depositional mineral associations in Precambrian iron-rich chemical sedimentary units may aid in the deconvolution of the redox record. Here, we present a case study and proposed workflow to decipher texturally early minerals from diagenetic indicators through the development of paragenetic sequence sets paired with texture-specific mineral and geochemical data. The focus will be on historic drill cores that transect Paleoproterozoic assemblages of Minnesota and Wisconsin (USA). Such units offer the opportunity to systematically decipher diagenetic heterogeneity. Key results include: (1) silicified horizons preserve multiple incomplete reaction sequences that can be deciphered into a relative order of events; (2) geochemical data separated from co-occurring banded and granular couplets record the same redox information for any given depth interval; and (3) iron-rich chemical sedimentary rocks may be reactive post-deposition, and so a full accounting of heterogeneity and local element mobility may need to be built into the larger diagenetic framework.

Geological Society of America Abstracts with Programs. Vol. 56, No. 3

doi: 10.1130/abs/2024NC-398797

© Copyright 2024 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.